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CHEM 1251 Fall 2024 Week 6 Problem Session PDF

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Summary

This document contains a problem session for a chemistry course, focusing on topics like solar cell efficiency, determining the frequency and energy of radiation, and calculations related to atomic properties and ionization. The session covers questions on atomic properties of elements, including determining trends in atomic size and ionization energies.

Full Transcript

# CHEM 1251 Fall 2024 - Week 6 Problem Session ## 1. Solar Cell Efficiency Of the sunlight that reaches Earth, roughly 7% lies in the ultraviolet region of the electromagnetic spectrum, 46% in the visible region, and 47% in the infrared region. Historically, solar cells only used visible waveleng...

# CHEM 1251 Fall 2024 - Week 6 Problem Session ## 1. Solar Cell Efficiency Of the sunlight that reaches Earth, roughly 7% lies in the ultraviolet region of the electromagnetic spectrum, 46% in the visible region, and 47% in the infrared region. Historically, solar cells only used visible wavelengths and the shortest of the IR wavelengths, but recently new designs have made use of longer IR wavelengths possible - increasing the efficiency of solar panels. The longest wavelength reported to be harvested by a solar cell is 1750 nm. **(a) Determine the frequency of this radiation.** * $c = \lambda \nu \implies \nu = \frac{c}{\lambda}$ * $\nu = \frac{3.00 \times 10^8 \text{ m/s}}{1.750 \times 10^{-6} \text{ m}} = 1.71 \times 10^{14} \text{ Hz}$ **(b) Determine the energy per photon of this radiation.** * $E = h\nu \implies E = \frac{hc}{\lambda}$ * $E = \frac{(6.63 \times 10^{-34} \text{ J s})(3.00 \times 10^8 \text{ m/s})}{1.75 \times 10^{-6} \text{ m}}$ * $E = 1.14 \times 10^{-19} \text{ J/photon}$ **(c) Determine the energy per mole of photons of this radiation.** * $E_{mol} = (1.14 \times 10^{-19} \text{ J/photon})(6.022 \times 10^{23} \text{ photons/mol})$ * $E_{mol} = 6.87 \times 10^4 \text{ J/mol}$ ## 2. Atomic Properties Determine which element has the greatest... **(a) Zeff.** * Ge: $Zeff = 32 - 28 = 4$ * Ca: $Zeff = 20 - 18 = 2$ * Se: $Zeff = 34 - 28 = 6$ **Answer: Se** **(b) Size.** * Atomic size increases as you move down and to the left on the periodic table. * Atomic size decreases as you move up and to the right. * $Zeff$ also affects size, with a higher $Zeff$ leading to a smaller radius due to the greater pull of the nucleus. **Answer: N** **(c) Average atomic mass.** **Answer: I** **(d) First ionization energy.** * First ionization energy increases as you move up and to the right. **Answer: He** **(e) First ionization energy.** * **Answer: S** * It is possible that N is the answer as well, as the trend for ionization energy is not strictly followed, but the general trend shows that S should have a greater ionization energy than Br. ## 3. Aluminum Ionization **(a) The first ionization energy of aluminum is 578 kJ/mol. How much energy, in J, is required to ionize one atom of Al?** * $578 \text{ kJ/mol} \times \frac{10^3 \text{ J}}{1 \text{ kJ}} \times \frac{1 \text{ mol}}{6.022 \times 10^{23} \text{ atoms}} = 9.60 \times 10^{-19} \text{ J}$ **(b) From which subshell is the electron ionized? Use the condensed electron configuration to help you describe this, and give the quantum numbers for this electron.** * Aluminum has a condensed electron configuration of $[Ne]3s^23p^1$ * Therefore, the electron that is ionized is in the 3p subshell. * The quantum numbers for that electron are: n=3, l=1, ml=0, s=+1/2 **(c) If it takes one photon with energy equal to or greater than the ionization energy to ionize an atom, what is the longest wavelength of light that would ionize aluminum?** * $E_{photon} = h\nu = \frac{hc}{\lambda}$ * $\lambda = \frac{hc}{E_{photon}} = \frac{(6.63 \times 10^{-34} \text{ J s})(3.00 \times 10^8 \text{ m/s})}{9.60 \times 10^{-19} \text{ J}} = 2.07 \times 10^{-7} \text{ m}$ **(d) It would take a photon of {higher | lower } wavelength to ionize silicon compared to aluminum. Explain:** * It would take a photon of **higher** wavelength to ionize silicon. * Ionization energy increases to the right on the periodic table, meaning silicon has a greater ionization energy than aluminum. * Because the energy of a photon is inversely proportional to its wavelength, a higher ionization energy means silicon would require a photon with lower wavelength (higher energy) to ionize. ## 4. Atomic Radius Ranking Arrange these atoms in order of increasing radius: * Ca, Rb, S, Si, Ge, F **Answer:** F, S, Si, Ge, Ca, Rb ## 5. Atomic and Ionic Radius Ranking Arrange these atoms or ions in order of increasing radius: * S<sup>2-</sup>, Ca<sup>2+</sup>, Cl<sup>-</sup>, K<sup>+</sup>, Ar * **Key points:** * Cations (positively charged ions) are smaller than their neutral atoms because they have lost an electron, making the remaining electrons more strongly attracted to the nucleus. * Anions (negatively charged ions) are larger than their neutral atoms because they have gained an electron, increasing the electron-electron repulsion, and making the electron cloud larger. **Answer:** Ca<sup>2+</sup>, K<sup>+</sup>, Ar, Cl<sup>-</sup>, S<sup>2-</sup> ## 6. Atomic and Ionic Radius Ranking Arrange these atoms or ions in order of increasing radius: * Br<sup>-</sup>, Br, I<sup>-</sup>, I, Kr * **Key points:** * Atomic radius increases going down and to the left on the periodic table. * Ions have different radii than neutral atoms based on the number of electrons they gain or lose. **Answer:** Kr, Br, Br<sup>-</sup>, I, I<sup>-</sup> ## 7. Copper Sphere Volume A pure copper sphere contains 8.62 x 10<sup>27</sup> electrons. What is the volume of the sphere in m<sup>3</sup>? Assume the sphere is made up of neutral copper atoms. The density of copper is 8.96 g/mL. * **Step 1:** Calculate the number of copper atoms. * Each copper atom has 29 electrons. * Number of copper atoms = (8.62 x 10<sup>27</sup> electrons) / (29 electrons/atom) = 2.97 x 10<sup>26</sup> atoms. * **Step 2:** Calculate the mass of the copper sphere. * Mass of copper atoms = (2.97 x 10<sup>26</sup> atoms) x (63.55 g/mol) / (6.022 x 10<sup>23</sup> atoms/mol) = 7.76 g. * **Step 3:** Calculate the volume of the copper sphere. * Density = Mass / Volume * Volume = Mass / Density = 7.76 g / (8.96 g/mL) = 0.866 mL * Convert mL to m<sup>3</sup>: 0.866 mL x (1 m<sup>3</sup> / 10<sup>6</sup> mL) = 8.66 x 10<sup>-7</sup> m<sup>3</sup> **Answer:** The volume of the copper sphere is 8.66 x 10<sup>-7</sup> m<sup>3</sup>.

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